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Protoplanetary accretion disks with coagulation and evaporation

โœ Scribed by Gregor E. Morfill


Publisher
Elsevier Science
Year
1988
Tongue
English
Weight
643 KB
Volume
75
Category
Article
ISSN
0019-1035

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๐Ÿ“œ SIMILAR VOLUMES


Evolution of Protoplanetary Disks with C
โœ Michael F. Sterzik; Gregor E. Morfill ๐Ÿ“‚ Article ๐Ÿ“… 1994 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 683 KB

We investigate the global evolution of the viscous stage of a turbulent protoplanetary disk. The time-dependent radial development of the nebula is calculated with the help of analytical onezone models of the vertical structure that relate optical properties of grains to turbulent viscosity. Special

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## Abstract A protoplanetary disk is a quasiโ€toroidal gasโ€“dust mixture rotating around a protostar that creates a complex intensity field in the internal disk medium in which planets are believed to form. In this work we start to model an idealized disk describing the radiation intensity propagatin